Quality of star images and determination of dimensions of the well-corrected field on plates of wide-angle astrographs.
The radius of the well-corrected field on a plate is determined from seeing estimates and measurement errors of stellar positions using different methods.
Kinematika i Fizika Nebesnykh Tel
- Pub Date:
- April 1985
- Image Analysis;
- Photographic Plates;
- Position Errors;
- Stellar Spectrophotometry;
- Image Processing;
- Northern Sky;
- Star Distribution;
- Wide Angle Lenses;
- Astrographs:Astronomical Optics;
- Astronomical Optics:Astrographs